Difference of Photometric Properties between Regular and Nonregular Miras in the Magellanic Clouds
Mira variables are asymptotic giant-branch pulsating stars with long pulsation periods and large amplitudes in optical bands. By applying the random forest algorithm to the I-band light curves for the Miras in the Magellanic Clouds, we have classified these Miras into regular Miras and nonregular Mi...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
American Astronomical Society
2022
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Online Access: | View Fulltext in Publisher |